LEADER 03832nam 22006375 450 001 9910257439503321 005 20200703133106.0 010 $a3-540-46397-6 024 7 $a10.1007/3-540-53059-2 035 $a(CKB)1000000000233565 035 $a(SSID)ssj0000326411 035 $a(PQKBManifestationID)12082548 035 $a(PQKBTitleCode)TC0000326411 035 $a(PQKBWorkID)10296434 035 $a(PQKB)10488715 035 $a(DE-He213)978-3-540-46397-9 035 $a(PPN)155231901 035 $a(EXLCZ)991000000000233565 100 $a20121227d1990 u| 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt 182 $cc 183 $acr 200 10$aRotation and Mixing in Stellar Interiors$b[electronic resource] $eProceedings of the Workshop Frontiers in Stellar Structure Theory, Held in Honor of Professor Evry Schatzman in Les Houches, France, June 19?25, 1989 /$fedited by Marie-Jo Goupil, Jean-Paul Zahn 205 $a1st ed. 1990. 210 1$aBerlin, Heidelberg :$cSpringer Berlin Heidelberg :$cImprint: Springer,$d1990. 215 $a1 online resource (XIII, 186 p. 6 illus.) 225 1 $aLecture Notes in Physics,$x0075-8450 ;$v366 300 $aBibliographic Level Mode of Issuance: Monograph 311 $a3-540-53059-2 327 $aRotation, lithium and mixing -- Surface abundances -- Stellar rotation prior to the main sequence -- The internal rotation of the sun -- Loss of mass and angular momentum: The observational point of view -- Pre-main sequence evolutionary tracks and lithium burning -- Mass transport and mixing by waves -- Turbulent transport in stratified and rotating fluids -- Penetration and overshooting from a convection zone -- Turbulent transport in stellar radiation zones: Causes and effects -- Will a magnetic field inhibit turbulent transport? -- Fast dynamo action-A critical problem for solar magnetism -- Observational constraints on the turbulent diffusion coefficient in late type stars -- Probing stellar interiors -- Conclusion. 330 $aThe 14 papers in this collection discuss recent progress in areas such as mixing in stellar interiors, redistribution and loss of angular momentum, emphasizing in particular the effects of turbulence. An introductory review by E. Schatzman, to whom this volume is dedicated, is followed by three sections: observational facts (surface abundances, stellar rotation, loss of mass and angular momentum, etc.), physical knowledge (mass transport and mixing by waves, turbulent transport, fast dynamo action, etc.), and the interpretation of observations. 410 0$aLecture Notes in Physics,$x0075-8450 ;$v366 606 $aObservations, Astronomical 606 $aAstronomy?Observations 606 $aAstrophysics 606 $aGeophysics 606 $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014 606 $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022 606 $aGeophysics/Geodesy$3https://scigraph.springernature.com/ontologies/product-market-codes/G18009 615 0$aObservations, Astronomical. 615 0$aAstronomy?Observations. 615 0$aAstrophysics. 615 0$aGeophysics. 615 14$aAstronomy, Observations and Techniques. 615 24$aAstrophysics and Astroparticles. 615 24$aGeophysics/Geodesy. 676 $a523.8 702 $aGoupil$b Marie-Jo$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aZahn$b Jean-Paul$4edt$4http://id.loc.gov/vocabulary/relators/edt 712 12$aWorkshop Frontiers in Stellar Structure Theory 906 $aBOOK 912 $a9910257439503321 996 $aRotation and Mixing in Stellar Interiors$92519167 997 $aUNINA